 It is radiating 24 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,824 K.

The secondary is a magnitude 10.24 star at an angular separation of from the primary along a position angle of 2°, as of 2015.The "Washington Double Star Catalog" (2001) notes this is an "optical pair, based on study of relative motion of the components," whereas Eggleton and Tokovinin (2008) list it as a binary system.Gaia Data Release 2 gives a parallax of for the companion, implying a distance around .